Impact of positrons on electrical conductivity of hot and dense astrophysical plasma

TL;DR

This paper investigates how positrons affect electrical conductivity in hot, dense astrophysical plasmas like neutron star crusts and white dwarf interiors, revealing that positron-induced collisions significantly influence transport properties.

Contribution

The study introduces positrons into the modeling of plasma conductivity and solves coupled kinetic equations with advanced collision calculations, providing new insights into plasma behavior.

Findings

Conductivity increases with temperature, following a T^4 law in semi-degenerate regimes.

Thermal electron-positron pair creation impacts collision rates and conductivity.

Positrons significantly influence transport properties in dense astrophysical plasmas.

Abstract

We study the influence of positrons on the outer crusts of neutron stars and the interiors of white dwarfs, introducing them as a novel component in both the composition of matter and in transport processes. We solve a system of coupled Boltzmann kinetic equations for the electron and positron distribution functions in the relaxation-time approximation, taking into account electron-ion, positron-ion, and electron-positron collisions. The relevant scattering matrix elements are calculated from one-plasmon exchange diagrams, with in-medium polarization tensors derived within hard-thermal-loop effective theory. Numerical results are obtained for matter composed of carbon nuclei. We find that the conductivity rises with temperature, following a power law sigma proportional to the 4th power of T in the semi-degenerate regime and sigma proportional to T in the nondegenerate regime, due to the intense creation of thermal electron-positron pairs and the resulting collisions among them. These results highlight the importance of including positrons in the transport properties of heated, dense astrophysical plasmas.